The period of the universe when the temperature of the universe had fallen enough that the strong force has separated but is high enough for the electromagnetic and weak force to remain merged into a single electroweak force is generally known as the electroweak epoch. It is generally considered as the start of the inflationary epoch, roughly between \(10^{-36}\)  seconds-\(10^{-32}\)  seconds after the Big Bang, [1]}, [2]}. The electroweak epoch ended with electroweak phase transition (EWPT). The nature of the phase transition can be of first order, second order or it can be a smooth crossover. The first order EWPT can be a source of gravitational waves, [3]}, [4]}. EWPT, in general, can not only be a potential candidate for baryogenesis if the Sakharov's conditions [5]} are satisfied but also can be a source to dilute the preexisting baryon asymmetry and the frozen out dark matter density by influx of entropy into the primeval plasma.
